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$\phi $ yield

From the 3$\gamma $ data sample, $\phi $ events are selected by requiring that there is no $\pi ^0$ in the event and that $\eta$ candidates from 2$\gamma $ pairs are constrained to $\pm10\%$ of the $\eta$ mass (0.5 $GeV/c_2 < M_{2\gamma} <$ 0.6 $GeV/c^2$). We do not require just the presence of the $\eta$ because $\pi ^0$ production is 50 times larger than $\eta$. Without cutting on the $\pi ^0$, the $\eta$ signal competes with the $\pi ^0$ combinatoric background. The invariant mass distribution of 3$\gamma $ is then formed for different minimum total energy in the LGD. These distributions for 4 different energy thresholds are shown in Fig. 1, where one can see how the $\phi $ peak becomes more prominent when the total energy threshold is increased.

The number of $\phi $ is found from the fit of these distributions to 3 Gaussians: one corresponding to the residual $\omega $ peak, one broad corresponding to the background (BG) and the third one for the $\phi $. To keep the number of parameters small, the position of the background Gaussian is set to be equal to the position of the $\omega $ peak, while the width of the BG is fixed to the $\omega $ width by $\sigma_{BG} = a \sigma_{\omega}$. In addition, the width of $\phi $ is kept constant during fitting, $\sigma_{\phi} = b$. Constants a and b are adjusted until good fits with reasonable looking background is found. Obtained $\phi $ mass, width and yield for different energy cuts are given in the Table 1.


Table 1: $\phi $ mass, width and yield as a function of minimum deposited energy in the LGD.
  $E_{TOT} > [Gev] $   $M_{\phi} [Gev/c^2]$   $\sigma_{\phi} [Gev/c^2]$  $N_{\phi}$
 3.5  0.931  0.065  555513.0
 4.0  0.943  0.065  460076.0
 4.5  0.954  0.070  228128.0
 5.0  0.967  0.075  87140.4

Figure 1: Three Gaussian fit in the limited interval of 3$\gamma $ invariant mass given by solid line. Dashed line is the sum of background and $\omega $ Gaussians.
\begin{figure}
\begin{center}\mbox{\epsfxsize =16.0cm\epsffile {phis.ps}}\end{center}\end{figure}


next up previous
Next: yield Up: gamma3 Previous: Introduction
Richard T. Jones 2004-04-30